Result for 0CBB9CB756DC7C6CC4F579A1F041D0F27FB92018

Query result

Key Value
FileName./usr/lib/aarch64-linux-gnu/cpl/plugins/hawki-2.4.3/hawki_detector_noise.la
FileSize1029
MD582FBE0762E9250394045A93FDE7CC631
SHA-10CBB9CB756DC7C6CC4F579A1F041D0F27FB92018
SHA-256CADDA848182C6E8F717815A90B10B023AF6D9BA75F3D7C7D5A9D23B4469B4F3D
SSDEEP24:nWeSGsWJjZmiVhhZRxIY+Ahmfvi4ivD2NGDe5/v0:neGsWJljXRxIY1hmfKxLcv0
TLSHT11111127FC39A613A6BD80B45568E306F428A40BA07551E5452C6CACF254BC1922B6E33
hashlookup:parent-total1
hashlookup:trust55

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Parents (Total: 1)

The searched file hash is included in 1 parent files which include package known and seen by metalookup. A sample is included below:

Key Value
FileSize470896
MD504E6CDD5BC92409B9B8ACCDBDA45598D
PackageDescriptionESO data reduction pipeline for the HAWK-I instrument This is the data reduction pipeline for the HAWK-I instrument of the Very Large Telescope (VLT) from the European Southern Observatory (ESO). . HAWK-I is a near-infrared (0.85-2.5 μm ) wide-field imager. It is being offered for the first time in Period 81. The instrument is cryogenic (120 K, detectors at 80 K) and has a full reflective design. The light passes four mirrors and two filter wheels before hitting a mosaic of four Hawaii 2RG 2048 * 2048 pixels detectors. The final F-ratio is F/4.36 ( 1 arcsec on the sky corresponds to 169 μm on the detector).
PackageMaintainerDebian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
PackageNamecpl-plugin-hawki
PackageSectionscience
PackageVersion2.4.3+dfsg-1
SHA-11AB820B4CF5A53A38486A13C3E51A928A2FE694D
SHA-256F4E93FD2283238717114016AB9CA5CDBD1B98D37FDA6784152CB5222AD3B3867